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Hybrid stars with large strange quark cores

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arxiv 2212.01132 v1 pith:L2OZRX2O submitted 2022-12-02 nucl-th astro-ph.HEhep-ph

Hybrid stars with large strange quark cores

classification nucl-th astro-ph.HEhep-ph
keywords quarkhybridlargepropertiesseveralstarscoresexistence
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The possible existence of hybrid stars is studied using several multi-quark interaction channels. The hadronic phase consists of an equation of state (EoS) with presently accepted nuclear matter properties and the quark model is constrained by the vacuum properties of several light mesons. The dependence of several NS properties on the different quark interactions is analyzed. We show that the present constraints from neutron star observations allow for the existence of hybrid stars with large strangeness content and large quark cores.

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